Low-mass Star Formation: Observations

被引：1

作者：

Evans, Neal J., II ^{[1
]}

机构：

[1] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA

来源：

COMPUTATIONAL STAR FORMATION | 2011年 / 270期

关键词：

stars: formation; infrared: ISM; submillimeter; YOUNG STELLAR OBJECTS; SPITZER SPECTROSCOPIC SURVEY; C2D LEGACY CLOUDS; DUST CONTINUUM EMISSION; MOLECULAR CLOUDS; GOULD BELT; EVOLUTIONARY SIGNATURES; PROTOSTELLAR ACCRETION; EPISODIC ACCRETION; ISOTHERMAL CLOUDS;

D O I：

10.1017/S1743921311000123

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

I briefly review recent observations of regions forming low mass stars. The discussion is cast in the form of seven questions that have been partially answered, or at least illuminated, by new data. These are the following: where do stars form in molecular clouds; what determines the IMP; how long do the, steps of the process take; how efficient; is star formation; do any theories explain the data; how are the star and disk built over time; and what chemical changes accompany star and planet formation. close with a summary and list of open questions.

引用

页码：25 / 32

页数：8

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